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<!DOCTYPE article SYSTEM "http://www.atmos-chem-phys-discuss.net/inc/acpd/copernicus.dtd">
<article language="en">
	<journal>
		<journal_title>Atmospheric Chemistry and Physics Discussions</journal_title>
		<journal_url>www.atmos-chem-phys-discuss.net</journal_url>
		<issn>1680-7367</issn>
		<eissn>1680-7375</eissn>
		<volume_number>4</volume_number>
		<issue_number>6</issue_number>
		<publication_year>2004</publication_year>
	</journal>
	<doi>10.5194/acpd-4-8141-2004</doi>
	<article_url>http://www.atmos-chem-phys-discuss.net/4/8141/2004/</article_url>
	<abstract_html>http://www.atmos-chem-phys-discuss.net/4/8141/2004/acpd-4-8141-2004.html</abstract_html>
	<fulltext_pdf>http://www.atmos-chem-phys-discuss.net/4/8141/2004/acpd-4-8141-2004.pdf</fulltext_pdf>
	<start_page>8141</start_page>
	<end_page>8170</end_page>
	<publication_date>2004-12-08</publication_date>
	<article_title content_type="html">Actinometric measurements of NO&lt;sub&gt;2&lt;/sub&gt; photolysis frequencies in the atmosphere simulation chamber SAPHIR</article_title>
	<authors>
		<author numeration="1" affiliations="1">
			<name>B. Bohn</name>
			<email>b.bohn@fz-juelich.de</email>
		</author>
		<author numeration="2" affiliations="1">
			<name>F. Rohrer</name>
		</author>
		<author numeration="3" affiliations="1">
			<name>T. Brauers</name>
		</author>
		<author numeration="4" affiliations="1">
			<name>A. Wahner</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Institut für Chemie und Dynamik der Geosphäre II: Troposphäre, Forschungszentrum Jülich, 52425 Jülich, Germany</affiliation>
	</affiliations>
	<abstract content_type="html">The simulation chamber SAPHIR at Forschungszentrum J&amp;#252;lich
has UV permeable teflon walls facilitating atmospheric
photochemistry studies under the influence of natural sunlight.
Because the internal radiation field is strongly affected by
construction elements, we use external, radiometric measurements
of spectral actinic flux and a model to calculate mean photolysis
frequencies for the chamber volume (Bohn and Zilken, 2004). In this work
we determine NO&lt;sub&gt;2&lt;/sub&gt; photolysis frequencies &lt;i&gt;j&lt;/i&gt;(NO&lt;sub&gt;2&lt;/sub&gt;) within
SAPHIR using chemical actinometry by injecting NO&lt;sub&gt;2&lt;/sub&gt; and
observing the chemical composition during illumination under
various external conditions. In addition to a photo-stationary
approach, a time-dependent method was developed to analyse the
data. These measurements had two purposes. Firstly, to check the
model predictions with respect to diurnal and seasonal variations
in the presence of direct sunlight and secondly to obtain an
absolute calibration factor for the combined radiometry-model
approach. We obtain a linear correlation between calculated and
actinometric &lt;i&gt;j&lt;/i&gt;(NO&lt;sub&gt;2&lt;/sub&gt;). A calibration factor of 1.34&amp;plusmn;0.10 is
determined, independent of conditions in good approximation. This
factor is in line with expectations and can be rationalised by
internal reflections within the chamber. Taking into account the
uncertainty of the actinometric &lt;i&gt;j&lt;/i&gt;(NO&lt;sub&gt;2&lt;/sub&gt;), an accuracy of 13%
is estimated for the determination of &lt;i&gt;j&lt;/i&gt;(NO&lt;sub&gt;2&lt;/sub&gt;) in SAPHIR. In
separate dark experiments a rate constant of
(1.93&amp;plusmn;0.12)&amp;times;10&lt;sup&gt;&amp;minus;14&lt;/sup&gt;&amp;nbsp;cm&lt;sup&gt;3&lt;/sup&gt;&amp;nbsp;s&lt;sup&gt;&amp;minus;1&lt;/sup&gt; was determined for
the NO+O&lt;sub&gt;3&lt;/sub&gt; reaction at 298 K using analytical and numerical
methods of data analysis.</abstract>
	<references>
	</references>
</article>

